A distinct material isolation and pole-to-pole teleconnection on Mars

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A distinct material isolation and pole-to-pole teleconnection on Mars | Research Square window.SnipcartSettings = { analytics: { enabled: false } }; (function() { var accessVector = localStorage.getItem('access_vector') || ''; window.dataLayer = window.dataLayer || []; if (accessVector) { window.dataLayer.push({ user: { profile: { profileInfo: { snid: accessVector } } } }); } })(); (function(w,d,s,l,i){w[l]=w[l]||[];w[l].push({'gtm.start':new Date().getTime(),event:'gtm.js'});var f=d.getElementsByTagName(s)[0],j=d.createElement(s),dl=l!='dataLayer'?'&l='+l:'';j.async=true;j.src='https://www.googletagmanager.com/gtm.js?id='+i+dl;f.parentNode.insertBefore(j,f);})(window,document,'script','dataLayer','GTM-K279D39R'); Browse Preprints In Review Journals COVID-19 Preprints AJE Video Bytes Research Tools Research Promotion AJE Professional Editing AJE Rubriq About Preprint Platform In Review Editorial Policies Our Team Advisory Board Help Center Sign In Submit a Preprint Cite Share Download PDF Article A distinct material isolation and pole-to-pole teleconnection on Mars Siteng Fan, Chen-Shuo Fan, Cong Sun, Zhiang Xie, Yangcheng Luo, and 1 more This is a preprint; it has not been peer reviewed by a journal. https://doi.org/ 10.21203/rs.3.rs-8056596/v1 This work is licensed under a CC BY 4.0 License Status: Under Review Version 1 posted You are reading this latest preprint version Abstract Global-scale circulation dominates material transport in planetary atmospheres, which is thought to account for large-scale compositional homogeneities on Earth and other planets. However, observations of the Martian atmosphere challenge this picture. The mixing ratios of dust and gas species (H 2 O, CO, Ar) show large planetary-scale inhomogeneities, yet the mechanism has been consistently overlooked. Here, we reveal and present that the coherent structure of the single-cell Hadley circulation on Mars can produce a distinct material transport pattern. It poses strong dynamical barriers that prevent material mixing, along with a special pole-to-pole teleconnection. Lagrangian particle tracking with reanalysis data suggests that the materials are isolated inside and outside the Hadley cell in the Martian atmosphere while connected between the two poles. Dimensional analysis indicates the reason to be a combined effect of the rapid planetary rotation and the thin atmosphere of Mars. The dominance of the mean circulation over the eddy transport gives rise to this unique transport regime, which is fundamentally distinct from those on Earth and Venus. This finding challenges the conventional view of material mixing of planetary-scale circulations, and presents a perspective of planetary atmospheric dynamics that confines materials and restricts redistributions. Earth and environmental sciences/Climate sciences/Atmospheric science/Atmospheric dynamics Earth and environmental sciences/Planetary science/Atmospheric dynamics Full Text Additional Declarations There is NO Competing Interest. Supplementary Files supplementary.figure.pdf Supplementary Figure supplementary.code.txt Supplementary Code supplementary.video.gif Supplementary Video Cite Share Download PDF Status: Under Review Version 1 posted You are reading this latest preprint version Research Square lets you share your work early, gain feedback from the community, and start making changes to your manuscript prior to peer review in a journal. As a division of Research Square Company, we’re committed to making research communication faster, fairer, and more useful. We do this by developing innovative software and high quality services for the global research community. Our growing team is made up of researchers and industry professionals working together to solve the most critical problems facing scientific publishing. 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